Zobrazeno 1 - 10
of 31
pro vyhledávání: '"M A, Brouwers"'
A significant fraction of white dwarfs show metal lines indicative of pollution with planetary material but the accretion process remains poorly understood. The main aim of this paper is to produce a road-map illustrating several potential routes for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f1b3623a92f5a22852591729a68692d9
http://arxiv.org/abs/2110.07601
http://arxiv.org/abs/2110.07601
The amount of nebular gas that a planet can bind is limited by its cooling rate, which is set by the opacity of its envelope. Accreting dust and pebbles contribute to the envelope opacity and, thus, influence the outcome of planet formation. Our aim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ab2a5e3dde34e848ff8f9f0d3336977
http://arxiv.org/abs/2106.03848
http://arxiv.org/abs/2106.03848
1. Introduction:In the traditional core accretion scenario, a planet grows by the subsequent accretion of a solid core and a gaseous envelope [3]. However, the accretion of these solids generates a large amount of heat, which can easily vaporize inco
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6df46ff5f6803d407610e88dda787545
https://doi.org/10.5194/epsc2020-1039
https://doi.org/10.5194/epsc2020-1039
Remnant paleodune deposits composed of carbonate and siliciclastic material are exposed slightly inland and along the Arabian Gulf coast of Abu Dhabi Emirate, United Arab Emirates. The paleodune deposits are here formally designated the Ghayathi Form
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e8c7774e039084f35c5a312e63661d06
https://doi.org/10.1201/9781003077862-14
https://doi.org/10.1201/9781003077862-14
Autor:
M. G. Brouwers, Chris W. Ormel
Proto-planets embedded in their natal disks acquire hot envelopes as they grow and accrete solids. This ensures that the material they accrete - pebbles, as well as (small) planetesimals - will vaporize to enrich their atmospheres. Enrichment modifie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::07026e6fcd026e3d084cfbe3db21c737
Publikováno v:
Astronomy & Astrophysics. 647:A175
During their formation, planets form large, hot atmospheres due to the ongoing accretion of solids. It has been customary to assume that all solids end up at the center constituting a "core" of refractory materials, whereas the envelope remains metal
Publikováno v:
Astronomy & Astrophysics, 611:A65. EDP Sciences
Context: Planet formation by pebble accretion is an alternative to planetesimal-driven core accretion. In this scenario, planets grow by accreting cm-to-m-sized pebbles instead of km-sized planetesimals. One of the main differences with planetesimal-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d54a530c8016dee1f21094b5bfa185c
Publikováno v:
Astronomy & Astrophysics. 621:C1
Autor:
Elise M. J. Brouwers-Kuyper, Peter M. A. van Ooijen, Edwin J. R. van Beek, Alfons H. H. Bongaerts, Matthijs Oudkerk, Piotr A. Wielopolski, Arie Berghout
Publikováno v:
The Lancet. 359:1643-1647
Diagnostic strategies for pulmonary embolism are complex and consist of non-invasive diagnostic tests done to avoid conventional pulmonary angiography as much as possible. We aimed to assess the diagnostic accuracy of magnetic resonance angiography (
Publikováno v:
Clinical radiology, 56(10), 838-842. W B SAUNDERS CO LTD
AIM: To determine the validity of a normal pulmonary angiogram in the exclusion of pulmonary embolism (PE), based on the safety of withholding anticoagulant therapy in patients with a normal pulmonary angiogram. MATERIALS AND METHODS: A review of Eng